Galactic Dynamics

Regular price €112.99
A01=James Binney
A01=Scott Tremaine
Amplitude
Angular momentum
Anisotropy
Approximation
Author_James Binney
Author_Scott Tremaine
Available energy (particle collision)
Azimuth
Boltzmann equation
Box orbit
Cartesian coordinate system
Category=PHVB
Center of mass
Circular orbit
Continuity equation
Dirac delta function
Dynamical friction
Eccentricity vector
Effective mass (solid-state physics)
Elliptical galaxy
eq_bestseller
eq_isMigrated=1
eq_isMigrated=2
eq_nobargain
eq_non-fiction
eq_science
Equation
Equations of motion
Escape velocity
Flatness problem
Free-fall time
Friedmann-Lemaitre-Robertson-Walker metric
Galactic Center
Galaxy rotation curve
Globular cluster
Gravitational field
Gravitational potential
Gravity
Harmonic oscillator
Hubble's law
Ideal gas
Impact parameter
Initial condition
Instability
Integral
Interstellar medium
Lagrangian point
Lambda-CDM model
Lindblad resonance
Main sequence
Mass distribution
Massive particle
Maxwell-Boltzmann distribution
Metallicity
N-body simulation
Number density
Orbital resonance
Phase space
Planetary nebula
Plummer model
Poisson's equation
Probability
Quantity
Quantum fluctuation
Relative velocity
Resonance
Rotational symmetry
Schwarzschild metric
Spherical model
Spheroid
Spiral galaxy
Star formation
Stellar classification
Stellar dynamics
Surface brightness
Toomre's Stability Criterion
Velocity dispersion
Virial theorem
WKB approximation

Product details

  • ISBN 9780691130279
  • Weight: 1276g
  • Dimensions: 152 x 235mm
  • Publication Date: 27 Jan 2008
  • Publisher: Princeton University Press
  • Publication City/Country: US
  • Product Form: Paperback
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Since it was first published in 1987, Galactic Dynamics has become the most widely used advanced textbook on the structure and dynamics of galaxies and one of the most cited references in astrophysics. Now, in this extensively revised and updated edition, James Binney and Scott Tremaine describe the dramatic recent advances in this subject, making Galactic Dynamics the most authoritative introduction to galactic astrophysics available to advanced undergraduate students, graduate students, and researchers. Every part of the book has been thoroughly overhauled, and many sections have been completely rewritten. Many new topics are covered, including N-body simulation methods, black holes in stellar systems, linear stability and response theory, and galaxy formation in the cosmological context. Binney and Tremaine, two of the world's leading astrophysicists, use the tools of theoretical physics to describe how galaxies and other stellar systems work, succinctly and lucidly explaining theoretical principles and their applications to observational phenomena. They provide readers with an understanding of stellar dynamics at the level needed to reach the frontiers of the subject. This new edition of the classic text is the definitive introduction to the field. * A complete revision and update of one of the most cited references in astrophysics * Provides a comprehensive description of the dynamical structure and evolution of galaxies and other stellar systems * Serves as both a graduate textbook and a resource for researchers * Includes 20 color illustrations, 205 figures, and more than 200 problems * Covers the gravitational N-body problem, hierarchical galaxy formation, galaxy mergers, dark matter, spiral structure, numerical simulations, orbits and chaos, equilibrium and stability of stellar systems, evolution of binary stars and star clusters, and much more * Companion volume to Galactic Astronomy, the definitive book on the phenomenology of galaxies and star clusters
James Binney is professor of physics at the University of Oxford. His books include "Galactic Astronomy". Scott Tremaine is the Richard Black Professor of Astrophysics at the Institute for Advanced Study and a member of the National Academy of Sciences. Both are fellows of the Royal Society.